Symmetries in the Hamiltonian formulation of string theory
arXiv:2406.14019 · doi:10.1155/ahep/6448068
Abstract
In the context of the Hamiltonian formulation of string theory, a widely acknowledged issue is the inability of the first-class constraints to accurately reproduce the Lagrangian symmetry transformations. We take a critical look at the Hamiltonian formulation of the Polyakov string and demonstrate, using Castellani's procedure, that diffeomorphism and Weyl symmetries naturally emerge without using any field-dependent reparametrization, thus preserving the theoretical consistency between Hamiltonian and Lagrangian descriptions. Additionally, we will review the standard Hamiltonian analysis of the symmetries in terms of lapse and shift functions and show that the reason behind this failure is not due to the non-canonicity of the variables but rather because this parametrization fails to preserve general covariance.
arXiv commentReferences are added, 11 pages; published version
References in corpus (9)
- Gauge transformations in the Lagrangian and Hamiltonian formalisms of generally covariant theories
- Hamiltonian Approach to Lagrangian Gauge Symmetries
- Master Equation for Lagrangian Gauge Symmetries
- The Hamiltonian formulation of General Relativity: myths and reality
- Diffeomorphism Invariance in the Hamiltonian formulation of General Relativity
- Gauge invariances vis-{á}-vis Diffeomorphisms in second order metric gravity: A new Hamiltonian approach
- Comments on BRST quantization of strings
- Diffeomorphism Symmetry in the Lagrangian Formulation of Gravity
- A new approach for nonrelativistic bosonic string in flat space time